Difference between revisions of "Workshop2022:rationale"
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ESA Gaia is continuing operations and is now well into its extended mission. In June 2022 Gaia consortium has released DR3 with a huge wealth of data products, including unprecedented astrometric, photometric and spectroscopic data. In the meantime, Gaia Photometric Science Alerts system continues its operation as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. | ESA Gaia is continuing operations and is now well into its extended mission. In June 2022 Gaia consortium has released DR3 with a huge wealth of data products, including unprecedented astrometric, photometric and spectroscopic data. In the meantime, Gaia Photometric Science Alerts system continues its operation as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. | ||
| − | === Gaia Alerts | + | === Science with Gaia Alerts === |
The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. | The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. | ||
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=== Follow-up and Time-Domain Astronomy === | === Follow-up and Time-Domain Astronomy === | ||
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In particular, for this workshop we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increasing the scientific output of surveys and follow-up observations in the multi-messenger era. | In particular, for this workshop we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increasing the scientific output of surveys and follow-up observations in the multi-messenger era. | ||
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=== Workshop's promise === | === Workshop's promise === | ||
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You are asked in the Registration to state your preference for in-person | You are asked in the Registration to state your preference for in-person | ||
| − | - if we are able to host that - or | + | - if we are able to host that - or online participation. We shall |
| − | certainly host | + | certainly host online participation. |
| − | Given the ever-changing Covid, travel | + | Given the ever-changing Covid, travel restrictions and post-travel |
quarantine requirements, we will make a final | quarantine requirements, we will make a final | ||
| − | decision on in-person participation in early | + | decision on in-person participation in early September. Individuals |
should follow their national guidance. | should follow their national guidance. | ||
For travel organising, please do ensure you have full | For travel organising, please do ensure you have full | ||
cancellation and health cover insurance in place. | cancellation and health cover insurance in place. | ||
Latest revision as of 14:14, 8 July 2022
Gaia and Gaia Alerts
ESA Gaia is continuing operations and is now well into its extended mission. In June 2022 Gaia consortium has released DR3 with a huge wealth of data products, including unprecedented astrometric, photometric and spectroscopic data. In the meantime, Gaia Photometric Science Alerts system continues its operation as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae.
Science with Gaia Alerts
The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses.
Follow-up and Time-Domain Astronomy
At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. The demand for time-domain observations of transients and other time-varying astrophysical phenomena is increasing and the Opticon-Radionet Pilot (ORP) community is trying to address this with its BHTOM virtual observatory.
In particular, for this workshop we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increasing the scientific output of surveys and follow-up observations in the multi-messenger era.
Workshop's promise
The forthcoming Gaia Alerts Workshop, the 13th in the series, will be an opportunity to learn about the current state of Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia DR3 and Gaia Alerts, and we will explore the scientific potential of Gaia.
During the workshop we will also explore the new possibilities offered by the Opticon-Radionet-Pilot H2020 in planning, obtaining and reducing in an efficient manner follow-up observations of transient alerts reported by other (non-GAIA) facilities.
Meeting in the Covid era
The successful experience of our previous meetings shows that working personal interactions are highly effective at developing plans, solving challenges, and extending partnerships to new participants. For that reason, we hope this can be primarily an in-person meeting and we should accommodate up to 50 attendees.
You are asked in the Registration to state your preference for in-person - if we are able to host that - or online participation. We shall certainly host online participation.
Given the ever-changing Covid, travel restrictions and post-travel quarantine requirements, we will make a final decision on in-person participation in early September. Individuals should follow their national guidance. For travel organising, please do ensure you have full cancellation and health cover insurance in place.
